M. R. Sanad
Articles written in Journal of Astrophysics and Astronomy
Volume 35 Issue 4 December 2014 pp 715-727
We present the ultraviolet spectra of two classical novae, BY Circini 1995 and V1425 Aquilae 1995, using observations obtained with the International Ultraviolet Explorer (IUE). The outflow velocity of the ionized ejecta was calculated to be 2100–2700 km s-1 and 1600–1900 km s-1 (FWHM) for BY Cir and V1425 Aql, respectively. The models generated by Jose & Hernanz (1998,
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